Search Publications

Identification of Kinetic Alfvén Wave Turbulence in the Solar Wind
DOI: 10.1088/2041-8205/745/1/L9 Bibcode: 2012ApJ...745L...9S

Bale, S. D.; Chen, C. H. K.; Mozer, F. S. +4 more

The nature of small-scale turbulent fluctuations in the solar wind is investigated using a comparison of Cluster magnetic and electric field measurements to predictions arising from models consisting of either kinetic Alfvén waves or whistler waves. The electric and magnetic field properties of these waves from linear theory are used to construct …

2012 The Astrophysical Journal
Cluster 266
Global model of lower band and upper band chorus from multiple satellite observations
DOI: 10.1029/2012JA017978 Bibcode: 2012JGRA..11710225M

Meredith, Nigel P.; Horne, Richard B.; Thorne, Richard M. +4 more

Gyroresonant wave particle interactions with whistler mode chorus play a fundamental role in the dynamics of the Earth's radiation belts and inner magnetosphere, affecting both the acceleration and loss of radiation belt electrons. Knowledge of the variability of chorus wave power as a function of both spatial location and geomagnetic activity, re…

2012 Journal of Geophysical Research (Space Physics)
Cluster DoubleStar 241
Large-scale electron acceleration by parallel electric fields during magnetic reconnection
DOI: 10.1038/nphys2249 Bibcode: 2012NatPh...8..321E

Egedal, J.; Daughton, W.; Le, A.

Magnetic reconnection is a process by which the field lines of a magnetized plasma undergo dramatic realignment, releasing large amounts of energy. Large-scale simulations of reconnection events in the Earth's magnetosphere suggest that this process takes place over much greater distances than previously expected.

2012 Nature Physics
Cluster 194
Local Kinetic Effects in Two-Dimensional Plasma Turbulence
DOI: 10.1103/PhysRevLett.108.045001 Bibcode: 2012PhRvL.108d5001S

Veltri, P.; Califano, F.; Servidio, S. +1 more

Using direct numerical simulations of a hybrid Vlasov-Maxwell model, kinetic processes are investigated in a two-dimensional turbulent plasma. In the turbulent regime, kinetic effects manifest through a deformation of the ion distribution function. These patterns of non-Maxwellian features are concentrated in space nearby regions of strong magneti…

2012 Physical Review Letters
Cluster 181
Particle Acceleration in the Magnetotail and Aurora
DOI: 10.1007/s11214-012-9874-4 Bibcode: 2012SSRv..173...49B

Zelenyi, L. M.; Baker, D. N.; Artemyev, A. V. +3 more

This paper deals with acceleration processes in the magnetotail and the processes that enhance particle precipitation from the tail into the ionosphere through electric fields in the auroral acceleration region, generating or intensifying discrete auroral arcs. Particle acceleration in the magnetotail is closely related to substorms and the occurr…

2012 Space Science Reviews
Cluster 180
Electric structure of dipolarization front at sub-proton scale
DOI: 10.1029/2012GL051274 Bibcode: 2012GeoRL..39.6105F

André, M.; Vaivads, A.; Huang, S. Y. +2 more

Using Cluster data, we investigate the electric structure of a dipolarization front (DF) - the ion inertial length (c/ωpi) scale boundary in the Earth's magnetotail formed at the front edge of an earthward propagating flow with reconnected magnetic flux. We estimate the current density and the electron pressure gradient throughout the D…

2012 Geophysical Research Letters
Cluster 179
Intermittent Dissipation at Kinetic Scales in Collisionless Plasma Turbulence
DOI: 10.1103/PhysRevLett.109.195001 Bibcode: 2012PhRvL.109s5001W

Matthaeus, W. H.; Chapman, S. C.; Daughton, W. +6 more

High resolution kinetic simulations of collisionless plasma driven by shear show the development of turbulence characterized by dynamic coherent sheetlike current density structures spanning a range of scales down to electron scales. We present evidence that these structures are sites for heating and dissipation, and that stronger current structur…

2012 Physical Review Letters
Cluster 164
Solar Wind Turbulent Spectrum at Plasma Kinetic Scales
DOI: 10.1088/0004-637X/760/2/121 Bibcode: 2012ApJ...760..121A

Maksimovic, M.; Alexandrova, O.; Mangeney, A. +2 more

The description of the turbulent spectrum of magnetic fluctuations in the solar wind in the kinetic range of scales is not yet completely established. Here, we perform a statistical study of 100 spectra measured by the STAFF instrument on the Cluster mission, which allows us to resolve turbulent fluctuations from ion scales down to a fraction of e…

2012 The Astrophysical Journal
Cluster 163
Occurrence rate of earthward-propagating dipolarization fronts
DOI: 10.1029/2012GL051784 Bibcode: 2012GeoRL..3910101F

André, M.; Vaivads, A.; Huang, S. Y. +2 more

The occurrence rate of earthward-propagating dipolarization fronts (DFs) is investigated in this paper based on the 9 years (2001-2009) of Cluster 1 data. For the first time, we select the DF events by fitting the characteristic increase in Bz using a hyperbolic tangent function. 303 earthward-propagating DFs are found; they have on ave…

2012 Geophysical Research Letters
Cluster 153
Pitch angle distribution of suprathermal electrons behind dipolarization fronts: A statistical overview
DOI: 10.1029/2012JA018141 Bibcode: 2012JGRA..11712221F

Daly, P. W.; André, M.; Vaivads, A. +5 more

We examine the pitch angle distribution (PAD) of suprathermal electrons (>40 keV) inside the flux pileup regions (FPRs) that are located behind the dipolarization fronts (DFs), in order to better understand the particle energization mechanisms operating therein. The 303 earthward-propagating DFs observed during 9 years (2001-2009) by Cluster 1 …

2012 Journal of Geophysical Research (Space Physics)
Cluster 148